The Space Life Sciences Training Program at Ames Research Center

The Space Life Sciences Training Program at Ames Research Center

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Space Life Sciences Training Program

An investment in tomorrow

The Space Life Sciences Training Program (SLSTP) provides undergraduate students entering their junior or senior years, and entering graduate students, with professional experience in space life science disciplines. This challenging ten-week summer program is hosted by NASA’s Ames Research Center in the heart of California’s Silicon Valley. The primary goal of the program is to train the next generation of scientists and engineers, enabling NASA to meet future research and development challenges in the space life sciences.

Summer 2023 SLSTP students at Ames Research Center.
Summer 2023 SLSTP students present their projects during midterm.
NASA / Stephanie Perreau Rainey

The SLSTP Experience
In this rigorous program, students work closely with renowned NASA scientists and engineers on cutting-edge research, benefitting from the concentration of bioscience expertise at Ames. In addition to conducting hands-on research, SLSTP students attend technical lectures given by experts on a wide range of topics and tour NASA research facilities.

This program provides opportunities for students to develop professional skills. These include technical and professional development training, presenting their scientific work and submitting an abstract to a professional scientific organization (e.g. the American Society for Gravitational and Space Research.)

SLSTP participants are exposed to a broad scope of space biosciences research performed by NASA scientists. While learning about the tools and methodology that enable biological experiments to be conducted in flight, students acquire skills and knowledge required for the design and execution of life science research conducted in microgravity.

Participants in the program receive a stipend and may be eligible to attend a scientific conference to formally present their research.

Research Areas
Students in SLSTP undertake research projects in multiple areas, including:

  • The effects of spaceflight on living systems, conducted both on the ground and also in space aboard the International Space Station and other spacecraft.
  • The development and operation of specialized research facilities to support investigations in microgravity, partial gravity, and hypergravity.
  • Research and development of advanced biotechnologies that enable NASA’s exploration of distant destinations.

Information for Applicants
The SLSTP is an equal opportunity program. Admission is by competitive application process. Past student participants were selected for their outstanding merit, passion for space, and desire to study space life science. Applicants must fulfill the following requirements: be a US citizen, age 18 or older in high academic standing (GPA of 3.2 or greater). Applicants should be junior or senior undergraduate student next Fall or a senior graduating in 2024 and entering graduate school for Fall 2024.

How to Apply:
Applications for the summer 2024 program will be opening soon in late 2023. Applications will be open in the NASA Internships Gateway portal.

SLSTP Mailing List
To subscribe to our mailing list and to receive e-mail announcements about the program and application process, please send an email to arc-slstp@mail.nasa.gov with “subscribe” in the subject to be added to our mailing list.

Program Support
The SLSTP is funded by NASA’s Space Biology Program, which is part of the Biological and Physical Sciences Division of NASA. The SLSTP is managed by the Space Biology Project within the Science Directorate at Ames Research Center.

For more information, contact:
arc-slstp@mail.nasa.gov

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Sonja Caldwell

Station Science 101: Microbiology

Station Science 101: Microbiology

astronaut Joe Acaba using an air sampling device inside the space station
NASA astronaut Joe Acaba with one of the Microbial Air Samplers, devices that monitor microbes in the air of the space station.
NASA

Wherever there are humans, there are microbes, too. Bacteria and fungi live all around us, in our homes, offices, industrial areas, the outdoors – even in space. People literally could not live without these tiny organisms, many of which are beneficial.

The trick is limiting potentially harmful ones, particularly in a contained environment such as a spacecraft. So from the launch of the very first module of the International Space Station, NASA has monitored its microbial community.

Because the station is an enclosed system, the only way that microbes get there is hitching a ride on the contents of resupply spacecraft from Earth and on arriving astronauts. The NASA Johnson Space Center Microbiology Laboratory puts a lot of effort into knowing which microbes ride along.

“We can’t sterilize everything we send into space, and don’t want to, but we do a lot to limit potential pathogens from making their way to the station,” says NASA microbiologist Sarah Wallace, Ph.D. “At launch, the cargo, food, vehicles, and crew members each have their own microbiome, or suite of microbes. When everything gets to the station, these microbiomes become part of the space station microbiome.”

The lab uses the traditional method of culturing a sample in a growth medium, similar to Petri dishes from high school science class, to sample a portion of everything during packing for launch and the launch vehicles themselves. This sampling confirms that contamination control plans are working properly – essentially making sure the numbers of microbes remain low and that those present are the ones normally expected.

bacteria culture inside space station
Astronauts sample a surface on the International Space Station for this microbial culture slide.
NASA

Then the lab continues monitoring after the vehicle, cargo, and crew arrive at the station. Crew members sample and culture microbes from the air, surfaces, and water on the station.

“It’s kind of a spot check to see how well housekeeping procedures are being implemented and how well the water system and the air filters are working,” Wallace says.

She calls the station’s water processing system “a phenomenal piece of engineering” that produces water much cleaner than most of us drink on Earth. In addition, the station itself is remarkably clean thanks to HEPA filters for the air and housekeeping practices for surfaces. “What microbes we see are really what we’d see if we looked at your home. In fact, we’ve done several studies comparing the station to a typical home and it is similar but usually cleaner,” she adds.

This monitoring over the lifetime of the orbiting lab has created a unique, long-term database that helps microbiologists know what to expect.

“Our requirements are two-fold, how much is there and what is there,” Wallace says. For years, the scientists didn’t know the ‘what’ until samples came back to ground. Now the equipment exists to perform direct swab-to-sequencer identification, eliminating the need to culture samples and return them to Earth. That equipment includes the miniPCR, a device that amplifies or makes many copies of a DNA strand using a process called polymerase chain reaction (PCR), and the MinION, a portable DNA sequencer. The Genes in Space 3 collaboration between Boeing and NASA paired these two platforms together, which led to the first identification of unknown bacteria off Earth.

NASA’s lab then conducted tests and confirmed that microbe identifications from the inflight process matched those determined on the ground down to the species level1.

“For the first time ever, we identified unknown microbes collected and cultured off Earth,” says Wallace. “We followed that up with the swab-to-sequencer, which lets us move away from culturing completely. We can swab a surface and sequence whatever is there.”

sample culture dishes inside the space station
Plates for culturing samples collected by the Microbial Air Samplers on the space station.
NASA

Subsequent work advanced the use of sequencing in space and later tests found that the culture-independent method showed the same microbial distributions as the standard culture-dependent method2. The swab-and-sequence method has been streamlined so that crew members can easily complete it in an extreme environment.

That is a critical capability for future missions to the Moon and Mars, both to continue to protect crew health and safety and to make sure that we do not contaminate other worlds. If explorers detect microbial life on another planet, they need to know whether it was already there or came from Earth.

Researchers also use the space station to conduct long-term microbial studies. The Microbial Tracking series studied what kinds of microbes are on the space station, both in the environment and in the astronauts’ bodies.

In addition to surveying the types of microbes present on the station, the lab studies whether those microbes could be harmful, as microgravity and radiation in space can render innocuous microorganisms potentially harmful and microbial behavior can change as the organisms adapt to the spaceflight environment.

So far, microbial issues on Earth far exceed any seen in space, Wallace says. “In addition to all the preflight monitoring, crew members are quarantined prior to launch. These steps were started back during Apollo missions and still are effective toward keeping our crews healthy.”

Because where people go, scientists want to know what microbes follow.

Citations

1 Burton AS, Stahl-Rommel SE, John KK, Jain M, Juul S, Turner DJ, Harrington ED, Stoddart D, Paten B, Akeson M, Castro-Wallace SL. Off Earth Identification of Bacterial Populations Using 16S rDNA Nanopore Sequencing. Genes. 2020 January 9; 76(11): 76 (https://www.mdpi.com/2073-4425/11/1/76)

2 Stahl-Rommel S, Jain M, Nguyen HN, Arnold RR, Aunon-Chancellor SM, Sharp GM, Castro CL, John KK, Juul S, Turner DJ, et al. Real-Time Culture-Independent Microbial Profiling Onboard the International Space Station Using Nanopore Sequencing. Genes. 2021; 12(1):106. (https://www.mdpi.com/2073-4425/12/1/106)

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55 Years Ago: Nine Months Before the Moon Landing

55 Years Ago: Nine Months Before the Moon Landing

In October 1968, the American human spaceflight program took significant steps toward achieving President John F. Kennedy’s goal of landing a man on the Moon and returning him safely to the Earth before the end of the decade. American astronauts returned to space after a 23-month hiatus. The success of the 11-day Apollo 7 mission heralded well for NASA to decide to send the next mission, Apollo 8, to orbit the Moon in December. The Saturn V rocket for that flight rolled out to its seaside launch pad two days before Apollo 7 lifted off. Preparations for later missions to test the Lunar Module (LM) in Earth orbit and around the Moon continued in parallel, as did work in anticipation of astronauts and their lunar samples returning from the Moon. Meanwhile, the Soviet Union also resumed its human spaceflight program.

Apollo 7 astronauts Donn F. Eisele,Walter M. Schirra, and R. Walter Cunningham review flight trajectories with Director of Flight Crew Operations Donald K. “Deke” Slayton shortly before launch Schirra, Eisele, and Cunningham suit up for launch Liftoff of Apollo 7, returning American astronauts to space
Left: Apollo 7 astronauts Donn F. Eisele, left, Walter M. Schirra, and R. Walter Cunningham review flight trajectories with Director of Flight Crew Operations Donald K. “Deke” Slayton shortly before launch. Middle: Schirra, left, Eisele, and Cunningham suit up for launch. Right: Liftoff of Apollo 7, returning American astronauts to space!

The liftoff of Apollo 7 astronauts Walter M. Schirra, Donn F. Eisele, and R. Walter Cunningham on Oct. 11, 1968, signaled the end of a 23-month hiatus in American human spaceflights resulting from the tragic Apollo 1 fire. To prevent a recurrence of the fire and to increase overall safety, NASA and North American Rockwell in Downey, California, redesigned the Apollo spacecraft, and Schirra, Eisele, and Cunningham spent months training to test it in Earth orbit. By the time they lifted off from Launch Pad 34 at NASA’s Kennedy Space Center (KSC) in Florida, the Saturn V rocket for the Apollo 8 mission had already rolled out to Launch Pad 39A a few miles away.

View of Apollo 7 lifting off from Launch Pad 34 The Apollo 7 S-IVB third stage, used as a rendezvous target Apollo 7 astronauts Donn F. Eisele, Walter M. Schirra, and R. Walter Cunningham on the prime recovery U.S.S. Essex
Left: View of Apollo 7 lifting off from Launch Pad 34, with the Saturn V for Apollo 8 on Launch Pad 39A in the background. Middle: The Apollo 7 S-IVB third stage, used as a rendezvous target. Right: Apollo 7 astronauts Donn F. Eisele, left, Walter M. Schirra, and R. Walter Cunningham on the prime recovery U.S.S. Essex following their successful 11-day mission.

During their 11-day mission, Schirra, Eisele, and Cunningham thoroughly tested the redesigned Apollo spacecraft. Early in the mission, they performed rendezvous maneuvers with their rocket’s S-IVB second stage, a maneuver planned for later missions to retrieve the LM. They thoroughly tested the Service Propulsion System engine, critical on later lunar missions for getting into and out of lunar orbit, by firing it on eight occasions, including the critical reentry burn to bring them home. The three astronauts conducted the first live television broadcasts from an American spacecraft, providing viewers on the ground with tours of their spacecraft. Teams from the U.S.S. Essex (CV-9) recovered Schirra, Eisele, and Cunningham and their Command Module (CM) from the Atlantic Ocean on Oct. 22. Apollo program managers declared that Apollo 7 “accomplished 101%” of its planned objectives. 

Apollo 8 astronauts James A. Lovell, William A. Anders, and Frank Borman attend the rollout of their Saturn V from the Vehicle Assembly Building to Launch Pad 39A The Apollo 8 Saturn V at Launch Pad 39A Borman, left, Lovell, and Anders pose with their Saturn V
Left: Apollo 8 astronauts James A. Lovell, left, William A. Anders, and Frank Borman attend the rollout of their Saturn V from the Vehicle Assembly Building to Launch Pad 39A. Middle: The Apollo 8 Saturn V at Launch Pad 39A. Right: Borman, left, Lovell, and Anders pose with their Saturn V following a crew egress exercise from their spacecraft.

The success of Apollo 7 gave NASA the confidence to announce in November that the next mission, Apollo 8, would attempt to enter orbit around the Moon. In early October, workers in High Bay 2 of KSC’s Vehicle Assembly Building (VAB) completed the stacking of the Saturn V rocket for Apollo 8 by adding the Command and Service Module (CSM). On Oct. 9, two days before Apollo 7 lifted off, as the Apollo 8 crew of Frank Borman, James A. Lovell, and William A. Anders and other NASA officials looked on, the completed Saturn V rolled out from the VAB to begin its eight-hour journey to Launch Pad 39A, three and a half miles away. After the rocket arrived at the pad and engineers began testing it, on Oct. 23, Borman, Lovell, and Anders suited up and practiced emergency egress from the spacecraft, as did their backups Neil A. Armstrong, Edwin E. “Buzz” Aldrin, and Fred W. Haise.

Apollo 8 astronauts Frank Borman, William A. Anders, and James A. Lovell on the deck of the M/V Retriever prepare for their water egress test Anders, Lovell, and Borman inside the boilerplate Apollo spacecraft during the water egress test Anders, Lovell, and Borman in the life raft after egressing from their spacecraft
Left: Apollo 8 astronauts Frank Borman, left, William A. Anders, and James A. Lovell on the deck of the M/V Retriever prepare for their water egress test. Middle: Anders, left, Lovell, and Borman inside the boilerplate Apollo spacecraft during the water egress test. Right: Anders, left, Lovell, and Borman in the life raft after egressing from their spacecraft.

As part of their training, Borman, Lovell, and Anders conducted water egress training in the Gulf of Mexico near Galveston, Texas. On Oct. 25, sailors aboard the Motor Vessel M/V Retriever lowered a mockup CM with the crew inside into the water in a nose-down position. Flotation bags inflated to right the spacecraft to a nose-up position. The astronauts then exited the capsule onto life rafts and recovery personnel hoisted them aboard a helicopter. The next day, backups Armstrong, Aldrin, and Haise repeated the test. 

Workers in the Vehicle Assembly Building at NASA’s Kennedy Space Center (KSC) in Florida lower the S-IVB third stage onto the S-II second stage during stacking operations of the Apollo 9 Saturn V Apollo 9 astronaut Russell L. Schweickart practices entering and leaving the Command Module while wearing a pressure suit during brief periods of weightlessness aboard a KC-135 aircraft Engineers conduct a docking test between the Apollo 9 CM, bottom, and Lunar Module in an altitude chamber in KSC’s Manned Spacecraft Operations Building
Left: Workers in the Vehicle Assembly Building at NASA’s Kennedy Space Center (KSC) in Florida lower the S-IVB third stage onto the S-II second stage during stacking operations of the Apollo 9 Saturn V. Middle: Apollo 9 astronaut Russell L. Schweickart practices entering and leaving the Command Module while wearing a pressure suit during brief periods of weightlessness aboard a KC-135 aircraft. Right: Engineers conduct a docking test between the Apollo 9 CM, bottom, and Lunar Module in an altitude chamber in KSC’s Manned Spacecraft Operations Building.

Preparations for Apollo 9 included training for the first spacewalk of the Apollo program. According to the mission plan, with the LM and CM docked, crew members in both spacecraft would open their hatches. During the spacewalk, one astronaut would transfer from the LM to the CM using handrails for guidance and enter the CM in a test of an emergency rescue capability. The training for this activity took place aboard a KC-135 aircraft from Patrick Air Force Base (AFB) in Florida. By flying repeated parabolic trajectories, the aircraft could simulate 20-30 seconds of weightlessness at a time, during which the astronauts wearing space suits practiced entering and exiting a mockup of the CM. Backup crew members Alan L. Bean and Richard F. Gordon completed the training on Oct. 9 followed by David R. Scott and Russell L. Schweickart of the prime crew the next day. North American Rockwell delivered the Apollo 9 CSM to KSC in early October. At the end the month, technicians in KSC’s Manned Spacecraft and Operations Building (MSOB) conducted a docking test of the Apollo 9 LM and CSM to verify the interfaces between the two vehicles. In the VAB’s High Bay 3, workers stacked the three stages of the Saturn V rocket for Apollo 9 during the first week of October.

Workers in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida uncrate the Apollo 10 Lunar Module (LM) descent stage shortly after its arrival MSOB workers unwrap the Apollo 10 LM ascent stage MSOB workers prepare to mate the Apollo 10 LM ascent stage to its descent stage
Left: Workers in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida uncrate the Apollo 10 Lunar Module (LM) descent stage shortly after its arrival. Middle: MSOB workers unwrap the Apollo 10 LM ascent stage. Right: MSOB workers prepare to mate the Apollo 10 LM ascent stage to its descent stage.

In preparation for Apollo 10, planned as a test of the CSM and LM in lunar orbit, the Grumman Aircraft Engineering Corporation in Bethpage, New York, delivered the LM for that mission to KSC. The descent stage arrived Oct. 11, followed by the ascent stage five days later. Technicians in the MSOB mated the two stages and installed the assembled vehicle into a vacuum chamber on Nov. 2 to begin a series of altitude tests.

A flight of the Lunar Landing Training Vehicle at Ellington Air Force Base in Houston The forward instrument panel of the Lunar Module Test Article-8 Richard Wright, administrative assistant for the Lunar Receiving Laboratory, gives astronaut Michael Collins a tour of the gloveboxes for examining lunar samples
Left: A flight of the Lunar Landing Training Vehicle at Ellington Air Force Base in Houston. Middle: The forward instrument panel of the Lunar Module Test Article-8. Right: Richard Wright, administrative assistant for the Lunar Receiving Laboratory, gives astronaut Michael Collins a tour of the gloveboxes for examining lunar samples.

The Lunar Landing Training Vehicle (LLTV), built by Bell Aerosystems of Buffalo, New York, allowed Apollo astronauts to master the intricacies of landing on the Moon by simulating the LM’s performance in the final few hundred feet of the descent to the surface. Although an excellent training tool, the LLTV and its predecessor the Lunar Landing Research Vehicle (LLRV) also carried some risk. Astronaut Armstrong ejected from an LLRV on May 6, 1968, moments before it crashed at Houston’s Ellington AFB. The final accident investigation report, issued on Oct. 17, cited a loss of helium pressure that caused depletion of the fuel used for the reserve attitude thrusters, with inadequate warning to the pilot as a contributing factor. By that time, Chief of Aircraft Operations Joseph S. “Joe” Algranti piloted the properly modified LLTV during its first flight on Oct 3. Algranti and NASA pilot H.E. “Bud” Ream completed 14 checkout flights before a crash in December grounded the LLTV. In October, NASA began a series of critical thermal-vacuum tests to certify the Apollo LM for lunar missions. The tests, conducted in the Space Environment Simulation Laboratory (SESL), at the Manned Spacecraft Center (MSC), now NASA’s Johnson Space Center in Houston, involved Grumman pilots Gerald P. Gibbons and Glennon M. Kingsley and astronaut James B. Irwin. The tests using Lunar Module Test Article-8, concluded in November, and simulated the temperatures expected during a typical flight to the Moon and descent to the surface.

To receive astronauts and their lunar samples after their return from the Moon, NASA built the Lunar Receiving Laboratory (LRL) in MSC’s Building 37. The LRL’s special design isolated astronauts and rock samples returning from the Moon to prevent back-contamination of the Earth by any possible lunar micro-organisms. By October 1968, with the Moon landing likely less than a year away, the LRL had reached a state of readiness that warranted a simulation of some its capabilities. Between Oct. 22 and Nov. 1, managers, scientists, and technicians carried out a 10-day simulation of LRL operations following a lunar landing mission. Although the exercise uncovered many deficiencies, enough time remained to correct them before the actual Moon landing.

Lift off of Soyuz 3 from the Baikonur Cosmodrome carrying cosmonaut Georgi T. Beregovoi Beregovoi during a television broadcast from Soyuz 3 The Soyuz 3 spacecraft carrying Beregovoi descends under its parachute for a soft-landing
Left: Lift off of Soyuz 3 from the Baikonur Cosmodrome carrying cosmonaut Georgi T. Beregovoi. Middle: Beregovoi during a television broadcast from Soyuz 3. Right: The Soyuz 3 spacecraft carrying Beregovoi descends under its parachute for a soft-landing. Image credits: courtesy Roscosmos.

As a reminder that a race to the Moon still existed, the Soviet Union also resumed crewed missions, halted in April 1967 by the death of Soyuz 1 cosmonaut Vladimir M. Komarov. Just three days after the Apollo 7 splashdown, the Soviets launched Soyuz 2, but without a crew. The next day, Soyuz 3 lifted off with cosmonaut Georgi T. Beregovoi aboard, at 47 the oldest person to fly in space up to that time. Although Beregovoi brought the two spacecraft close together, he could not achieve the intended docking. Soyuz 2 landed on Oct. 28 and Beregovoi in Soyuz 3 two days later. Following the Zond 5 circumlunar flight in September, rumors persisted that the next Zond mission may soon carry two cosmonauts on a similar circumlunar flight. The apparently successful Zond 5 mission coupled with the rumors of an imminent Soviet crewed lunar mission possibly contributed to the decision to send Apollo 8 on its historic circumlunar flight in December 1968.

News from around the world in October 1968:

Oct. 2 – Redwood National Park established to preserve the tallest trees on Earth.

Oct. 7 – The Motion Picture Association of America adopts a film rating system.

Oct. 12 – Equatorial Guinea gains independence from Spain.

Oct. 12 – The XIX Olympic Games open in Mexico City, the first time the games held in Latin America.

Oct. 14 – The Beatles finish recording the double “White Album.”

Oct. 16 – The Jimi Hendrix Experience releases its last studio album “Electric Ladyland.”

Oct. 17 – Release of the film “Bullitt,” starring Steve McQueen.

Oct. 20 – American high jumper Dick Fosbury introduces the Fosbury Flop technique at the Mexico City Olympics.

Oct. 24 – The 199th and last flight of the X-15 hypersonic rocket plane takes place at Edwards Air Force Base in California, piloted by NASA pilot William H. Dana.

Oct. 25 – Led Zeppelin gives its first concert, at Surrey University in England.

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Kelli Mars

International Ocean Satellite Monitors How El Niño Is Shaping Up

International Ocean Satellite Monitors How El Niño Is Shaping Up

The maps above show sea levels in the Pacific Ocean
The maps above show sea levels in the Pacific Ocean during early October of 1997, 2015, and 2023, in the run up to El Niño events. Higher-than-average ocean heights appear red and white, and lower-than-average heights are in blue and purple.
NASA/JPL-Caltech

Sentinel-6 Michael Freilich is the latest satellite contributing to a 30-year sea level record that researchers are using to compare this year’s El Niño with those of the past.

Not all El Niño events are created equal. Their impacts vary widely, and satellites like the U.S.-European Sentinel-6 Michael Freilich help anticipate those impacts on a global scale by tracking changes in sea surface height in the Pacific Ocean.

Water expands as it warms, so sea levels tend to be higher in places with warmer water. El Niños are characterized by higher-than-normal sea levels and warmer-than-average ocean temperatures along the equatorial Pacific. These conditions can then propagate poleward along the western coasts of the Americas. El Niños can bring wetter conditions to the U.S. Southwest and drought to regions in the western Pacific, including Indonesia. This year’s El Niño is still developing, but researchers are looking to the recent past for clues as to how it is shaping up.

There have been two extreme El Niño events in the past 30 years: the first from 1997 to 1998 and the second from 2015 to 2016. Both caused shifts in global air and ocean temperatures, atmospheric wind and rainfall patterns, and sea level. The maps above show sea levels in the Pacific Ocean during early October of 1997, 2015, and 2023, with higher-than-average ocean heights in red and white, and lower-than-average heights in blue and purple. Sentinel-6 Michael Freilich captured the 2023 data, the TOPEX/Poseidon satellite collected data for the 1997 image, and Jason-2 gathered data for the 2015 map.

By October 1997 and 2015, large areas of the central and eastern Pacific had sea levels more than 7 inches (18 centimeters) higher than normal. This year, sea levels are about 2 or 3 inches (5 to 8 centimeters) higher than average and over a smaller area compared to the 1997 and 2015 events. Both of the past El Niños reached peak strength in late November or early December, so this year’s event may still intensify.

“Every El Niño is a little bit different,” said Josh Willis, Sentinel-6 Michael Freilich project scientist at NASA’s Jet Propulsion Laboratory in Southern California. “This one seems modest compared to the big events, but it could still give us a wet winter here in the Southwest U.S. if conditions are right.”

More About the Mission

Launched in November 2020, Sentinel-6 Michael Freilich is named after former NASA Earth Science Division Director Michael Freilich. The satellite is one of two that compose the Copernicus Sentinel-6/Jason-CS (Continuity of Service) mission.

Sentinel-6/Jason-CS was jointly developed by ESA (European Space Agency), the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT), NASA, and the U.S. National Oceanic and Atmospheric Administration, with funding support from the European Commission and technical support on performance from the French space agency CNES (Centre National d’Études Spatiales).

To learn more about Sentinel-6 Michael Freilich, visit:

https://www.nasa.gov/sentinel-6

News Media Contacts

Jane J. Lee / Andrew Wang
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-0307 / 626-379-6874
jane.j.lee@jpl.nasa.gov / andrew.wang@jpl.nasa.gov

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Anthony Greicius

NASA Employees Win Top Federal Award for Asteroid Deflection Mission

NASA Employees Win Top Federal Award for Asteroid Deflection Mission

Scott Bellamy, left, and Brian Key, right, stop for a photo moments after receiving the Samuel J. Heyman Service to America Medals. Bellamy and Key accepted on behalf of the entire DART team during a ceremony at the John F. Kennedy Center for Performing Arts in Washington on Oct. 17.
Scott Bellamy, left, and Brian Key, right, received the Samuel J. Heyman Service to America Medals. Bellamy and Key accepted on behalf of the entire DART team during a ceremony at the John F. Kennedy Center for Performing Arts in Washington on Oct. 17.
Allison Shelley for the Partnership for Public Service

NASA’s Brian Key and Scott Bellamy accepted the Samuel J. Heyman Service to America Medal on behalf of a mission team for the first planetary defense test during a ceremony at the John F. Kennedy Center for Performing Arts in Washington on Oct. 17.

The awards program for career federal employees, known as the Sammies, aims to highlight key accomplishments that benefit the nation, seeks to build trust in government, and inspire people to consider careers in public service.

Known as DART, NASA’s Double Asteroid Redirection Test mission successfully impacted a known asteroid in September 2022 and altered its orbit, demonstrating one planetary defense method that could be used to protect Earth from a potentially hazardous asteroid on a collision course with our home planet if one were ever discovered.

Key and Bellamy served as program manager and mission manager for DART, respectively, and are based in the Planetary Missions Program Office at NASA’s Marshall Space Flight Center in Huntsville, Alabama. For their work on the mission, the team was honored in the Science, Technology, and Environment category of the Heyman awards.

“DART was a first-of-its-kind mission that marked a watershed moment for planetary defense. The DART team members are some of the very best of NASA, and we are so excited to see Brian Key and Scott Bellamy recognized for their contributions and leadership,” NASA Administrator Bill Nelson said. “Brian, Scott, and the entire DART team have shaped the course of human space exploration, inspiring people around the world through innovation. Thanks to their dedication and hard work, NASA is better prepared to defend our home planet, and will be ready for whatever the universe throws at us.”

In his role on DART, Key maintained budget, staff, and schedule oversight for the mission and worked directly with DART spacecraft developers at Johns Hopkins Applied Physics Laboratory in Laurel, Maryland.

“I’m elated to see our team honored with this award and hope it will bring more attention to the valuable work NASA does to defend our home world,” Key said, who oversees management of NASA’s $2 billion portfolio spanning the Discovery Program, the New Horizons Program, and the Solar System Exploration Program, which covers the full range of large and small science missions exploring the planets, moons, asteroids, comets and other destinations of interest in the solar system.

Bellamy was tasked with keeping the team on track to launch and operate the mission. He echoed Key’s praise for the entire DART team.

“We’re just the managers,” Bellamy said. “Our role has been to serve the team, keeping things moving forward as smoothly as possible to enable them to do the actual hands-on, pencilwork-to-hardware that brought this mission from concept to reality.”

That mission could not have gone more flawlessly, they agreed. Launched in November 2021, the DART spacecraft traveled to more than 6.8 million miles from Earth with one simple goal: to intentionally impact into Dimorphos, a 492-foot-diameter asteroid, at roughly 14,000 miles per hour, thus altering its orbit around its much larger parent asteroid, Didymos. DART’s collision with Dimorphos altered the asteroid’s roughly 12-hour orbit period around its parent by about a half-hour.

“I don’t even have the words to describe the release of emotion in the control room when we got confirmation that DART had impacted,” Bellamy said. “The whole team went from nail-biting suspense to unbelievable excitement in a matter of seconds.”

As for future planetary defense activities, NASA and its partners will build on DART’s success. A follow-up mission by ESA (European Space Agency), called Hera, is scheduled to launch in 2024 to further assess DART’s impact on Dimorphos. NASA also is developing the NEO Surveyor mission, which is designed to accelerate the rate at which the agency can discovery potentially hazardous near-Earth objects, asteroids and comets which can come close to Earth and could pose an impact risk.

Johns Hopkins Applied Physics Laboratory managed the DART mission for NASA’s Planetary Defense Coordination Office. The agency provided support for the mission from several centers, including the Jet Propulsion Laboratory in Southern California; Goddard Space Flight Center in Greenbelt, Maryland; NASA’s Johnson Space Center in Houston; Glenn Research Center in Cleveland; and Langley Research Center in Hampton, Virginia.

Learn more about NASA’s Planetary Missions Program and Planetary Defense Coordination Offices online.

-end-

News Media Contacts

Jackie McGuinness
Headquarters, Washington
202-358-1600
jackie.mcguinness@nasa.gov

Jonathan Deal
Marshall Space Flight Center, Huntsville, Ala.
256-544-0034
jonathan.e.deal@nasa.gov

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Last Updated

Oct 18, 2023

Editor

Claire A. O’Shea

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Claire A. O’Shea